2020
DOI: 10.1134/s0020168520050131
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X-ray Photoelectron Spectroscopy Study of Indium Tin Mixed Oxides on the Surface of Silicate Glass

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Cited by 17 publications
(12 citation statements)
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“…30 Furthermore, the larger peak at 17.5 eV, labeled in Figure 5a as In-17.5, denotes either the binding energy of In 0 (In 4d 5/2 ) in the alloy (galinstan), shifted to higher binding energies due to alloying (with Ga), 30 or indium oxides, 31 for instance, in indium tin mixed oxides. 32 We assume that the peak at 17.5 eV denotes indium oxide, which may stem from a buried layer of oxidized indium buried below the gallium oxide. 33 The presence of pure element Ga 0 is proven by the presence of Ga 3d 5/2 at 18.6 eV, 34 albeit the peak area is smaller than that of the indium oxide peak (In 4d 5/2 ).…”
Section: ■ Results and Discussionmentioning
confidence: 99%
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“…30 Furthermore, the larger peak at 17.5 eV, labeled in Figure 5a as In-17.5, denotes either the binding energy of In 0 (In 4d 5/2 ) in the alloy (galinstan), shifted to higher binding energies due to alloying (with Ga), 30 or indium oxides, 31 for instance, in indium tin mixed oxides. 32 We assume that the peak at 17.5 eV denotes indium oxide, which may stem from a buried layer of oxidized indium buried below the gallium oxide. 33 The presence of pure element Ga 0 is proven by the presence of Ga 3d 5/2 at 18.6 eV, 34 albeit the peak area is smaller than that of the indium oxide peak (In 4d 5/2 ).…”
Section: ■ Results and Discussionmentioning
confidence: 99%
“…A peak at a binding energy of 16.5 eV is visible, which denotes pure In 0 (In 4d 5/2 ) . Furthermore, the larger peak at 17.5 eV, labeled in Figure a as In-17.5, denotes either the binding energy of In 0 (In 4d 5/2 ) in the alloy (galinstan), shifted to higher binding energies due to alloying (with Ga), or indium oxides, for instance, in indium tin mixed oxides . We assume that the peak at 17.5 eV denotes indium oxide, which may stem from a buried layer of oxidized indium buried below the gallium oxide .…”
Section: Resultsmentioning
confidence: 99%
“…To avoid possible peak shifts due to charging, the binding energies of the XPS spectra were corrected by setting the maximum of the adventitious carbon peak in the C 1s spectra to 284.4 eV. The assignment of the peaks relied on several literatures. ,, We acknowledge that the assignment of different chemical states of nickel oxide is quite complex in XPS; however, in this case, there was no detectable change in the shape of Ni 2p spectra with or without MeO-2PACz but rather a peak shift. Hence, we believed that the assignment sufficed for the purpose of elemental identification of our thin layers.…”
Section: Methods Sectionmentioning
confidence: 99%
“…In contrast to the pristine sample, here the intensity of Sb 2 O 3 is relatively lower than InSb, implying that some portion of oxidized Sb participates in the magnesiation reaction, as already observed for surface tin oxides [ 37 , 41 ], or reacts with the electrolyte. Surprisingly, a broad peak corresponding to In(OH) 3 is observed around 533.0 eV), which might arise from a parasitic and irreversible chemical reaction between discharged InSb and the THF solvent [ 56 , 57 ]. On further discharge (½D1 and D1), all the peaks related to pristine components vanish, while a new doublet corresponding to the Mg 3 Sb 2 (526.8, 536.2 eV) compound appears (reference spectra of Mg 3 Sb 2 are given in Figure S1 ).…”
Section: Resultsmentioning
confidence: 99%